On the Explosion Mechanism of SNe Type Ia
arXiv:astro-ph/0111473 · doi:10.1016/S1387-6473(02)00187-2
Abstract
In this article we discuss the first simulations of two- and three-dimensional Type Ia supernovae with an improved hydrodynamics code. After describing the various enhancements, the obtained results are compared to those of earlier code versions, observational data and the findings of other researchers in this field.
7 pages, 4 figures
References in corpus (1)
Cited by in corpus (9)
- Carbon Ignition in Type Ia Supernovae: An Analytic Model
- Full-star Type Ia supernova explosion models
- Following multi-dimensional Type Ia supernova explosion models to homologous expansion
- Type Ia supernova diversity in three-dimensional models
- Multi-spot ignition in type Ia supernova models
- The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in Type Ia supernovae
- Detectibility of Mixed Unburnt C+O in Type Ia Supernova Spectra
- Detailed Spectral Modeling of a 3-D Pulsating Reverse Detonation Model: Too Much Nickel
- Multi-dimensional numerical simulations of type Ia supernova explosions